Home Page Updated on December 16, 2020
MisV0854
|
R.A. | 17h00m39s.75 | |
Decl. | -30o10'51".5 | (2000.0) |
Mag. | 12.4-14.2C | |
Type | SR: |
= USNO-A2.0_0525.25571476 17 00 39.749 -30 10 51.54 17.5R 20.6B
Digitized Sky Survey GIF image (15 x 15 arcmin)
It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ken-ichi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida.
OW Oph is 1.7 arcmin from MisV0854, that was detected as a variable star between 10.8 - 13.4 mag. MisV0854 is thus a new variable star.
12.3 +--------------------------------------------------------+ | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | * | | | | | | * | 14.3 +--------------------------------------------------------+ 2451267 2451615 1999 Mar. 29 2000 Mar. 11
Date | Mag | Filter | Observer |
---|---|---|---|
1999 Apr. 14.72598 | 13.9 | C | Ken-ichi Kadota |
1999 Apr. 14.72655 | 13.9 | C | Ken-ichi Kadota |
1999 June 14.55856 | 14.2 | C | Ken-ichi Kadota |
2000 Feb. 24.81377 | 12.4 | C | Ken-ichi Kadota |
2000 Feb. 24.81433 | 12.4 | C | Ken-ichi Kadota |